Tilted homogeneous cosmological models

Details Tilted homogeneous cosmological models Tilted homogeneous cosmological models

Sep 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973cmaph..31..209k&link_type=abstract

Communications in Mathematical Physics, Volume 31, Issue 3, pp.209-242

Mathematics

Mathematical Physics

168

Scientific paper

We examine spatially homogeneous cosmological models in which the matter content of space-time is a perfect fluid, and in which the fluid flow vector is not normal to the surfaces of homogeneity. In such universes, the matter may move with non-zero expansion, rotation and shear; we examine the relation between these kinematic quantities and the Bianchi classification of the symmetry group. Detailed characterizations of some of the simplest such universe models are given.

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